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Now showing items 11-17 of 17
Alpha and neutron induced reactions on ruthenium
(2001-05-21)
Measurement of the (gamma,n) reaction rates of the nuclides Pt-190, Pt-192, and Pt-198 in the astrophysical gamma process
(2001-05)
The nucleosynthesis of heavy neutron-deficient nuclei in a stellar photon bath at the temperatures relevant for the astrophysical gamma process was investigated. In order to derive (gamma ,n) cross sections and reaction ...
End point of the rp process on accreting neutron stars
(2001-04-16)
We calculate the rapid proton (rp) capture process of hydrogen burning on the surface of an accreting neutron star with an updated reaction network that extends up to Xe, far beyond previous work. In both steady-state ...
Nucleosynthesis in massive stars using extended adaptive nuclear reaction networks
(American Institute of Physics (AIP), 2001)
We present the first calculations to follow the evolution of all stable isotopes and their abundant radioactive progenitors in a finely zoned stellar model from the onset of central hydrogen burning through explosion as a ...
Element synthesis in stars
(Elsevier, 2001)
Except for H-1, H-2, He-3, He-4, and Li-7, originating from the Big Bang, all heavier elements are made in stellar evolution and stellar explosions. Nuclear physics, and in many cases nuclear structure far from stability, ...
Nuclear aspects of stellar and explosive nucleosynthesis
(Springer Nature, 2001)
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not yet fully accessible by experiments. Therefore, there is high demand for reliable predictions of cross sections and reaction rates by ...